Pith. sign in

REVIEW 2 cited by

Cosmology with the Square Kilometre Array by SKA-Japan

Not yet reviewed by Pith; the record is open.

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 1603.01959 v3 pith:DIEES4GV submitted 2016-03-07 astro-ph.CO

classification astro-ph.CO
keywords cosmologyarraybeencosmologicalfundamentalkilometreprecisionquestions
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

In the past several decades, the standard cosmological model has been established and its parameters have been measured to a high precision, while there are still many of the fundamental questions in cosmology; such as the physics in the very early Universe, the origin of the cosmic acceleration and the nature of the dark matter. The future world's largest radio telescope, Square Kilometre Array (SKA), will be able to open the new frontier of cosmology and will be one of the most powerful tools for cosmology in the next decade. The cosmological surveys conducted by the SKA would have the potential not only to answer these fundamental questions but also deliver the precision cosmology. In this article we briefly review the role of the SKA from the view point of the modern cosmology. The cosmology science led by the SKA-Japan Consortium (SKA-JP) Cosmology Science Working Group is also discussed.

Discussion (0). Continue with ORCID to comment.

Forward citations

Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Redshift space distortions in the presence of non-minimally coupled dark matter

    astro-ph.CO 2019-08 conditional novelty 6.0 of 10

    In dark matter-dark energy coupling models, the Kaiser formula gains a coupling-dependent term, so redshift-space distortions measure an effective growth rate that differs from the true matter growth rate, with Euclid...

  2. Probing initial isocurvature perturbation with 21cm one-point statistics

    astro-ph.CO 2025-09 conditional novelty 5.0 of 10

    A Fisher forecast from 21cmFAST simulations shows 21cm variance can constrain the CDM isocurvature fraction to about 3e-4 with SKA, while skewness is an order of magnitude weaker.

Pith tools